We investigate the global evolution of the viscous stage of a turbulent protoplanetary disk. The time-dependent radial development of the nebula is calculated with the help of analytical onezone models of the vertical structure that relate optical properties of grains to turbulent viscosity. Special
โฆ LIBER โฆ
Protoplanetary accretion disks with coagulation and evaporation
โ Scribed by Gregor E. Morfill
- Publisher
- Elsevier Science
- Year
- 1988
- Tongue
- English
- Weight
- 643 KB
- Volume
- 75
- Category
- Article
- ISSN
- 0019-1035
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## Abstract A protoplanetary disk is a quasiโtoroidal gasโdust mixture rotating around a protostar that creates a complex intensity field in the internal disk medium in which planets are believed to form. In this work we start to model an idealized disk describing the radiation intensity propagatin